2017년 1월 3일 화요일

ショルツ star

ショルツ star

WISE J072003.20-084651.2[1]
Temporary mark, another name 2MASS J07200325-0846499
Constellation Monoceros
Apparent magnitude (V) 18.3[2]
Classification Binary system of a red dwarf and the brown dwarf
Discovery
Detector Ralf-Dieter Scholz
Discovery method From an observation result of WISE
Position
Epoch: J2000.0
Right ascension (RA,α) 07h 20m 03.254s [1]
Declination (Dec,δ) -08° 46′ 49.90″ [1]
Radial velocity (Rv) 83.1 km/s[2]
Proper motion (μ) Right ascension: -36 milliseconds / year [1]
Declination: -102 milliseconds / year [1]
Annual parallax (π) 166+-28 milliseconds
Absolute magnitude (MV) 19.4[3]
Physical property
Mass 0.15M[2]
Spectral class M9 +-1 [2]
T5[2]
Age 3,000,000,000-10,000,000,000 years [2]
The other name
The other name
Scholz's Star,[4] Scholz's star,[2] WISE J072003.20-084651.2,[1] WISE 0720-0846, 2MASS J07200325-0846499,[1] 2MASS 0720-0846
■Project ■ Template

A ショルツ star [5] (Scholz's Star, another name WISE 0720-0846, WISE J072003.20-084651.2[4]) I belong to とは, Monoceros and am binary system in the distance of 17-23 light-year (5.1-7.2 parsec) from the solar system [2].

Table of contents

Summary

The main star of the binary system is spectral class M9 +-1, and mass is a red dwarf of the 86+-2 Jupiter mass [2], and probably the subordinate star is a brown dwarf of the T5 type, and mass is 65+-12 Jupiter mass [2]. It becomes the 0.15 sun mass in the whole binary system [2]. Approximately 0.8 au [2], the apparent class of the binary system are 18.3 [2] and do not show the distance between both heavenly bodies by the naked eye. The age is calculated from 30 with 10 billion years [2]. 80 stars system is to exist than this system near the sun when I estimate distance as 166 milliseconds angle in annual parallax of this binary system [6].

Discovery

As for what these heavenly bodies discovered when the sun was a fixed star of neighboring, [4], the study were published in arXiv in astronomer Ralph = Dieter ショルツ (Ralf-Dieter Scholz) of Potsdam heavenly bodies physics laboratory (AIP) in November, 2013. These heavenly bodies came to be called by a nickname of "ショルツ star" (Scholz's Star) afterwards.

Approach with the solar system

When the ショルツ star system passed the distance of 52,000 aus (0.25 parsec, 0.82 light-year) now from the sun approximately 70,000 years ago, is calculated [2]; [4]. This distance is the outside domain of the cloud of オールト assumed as the origin of a long periodic comet and the non-periodic comet. In addition, a comet is temporarily said from a cloud of オールト under the influence of ショルツ star system even if scattered that I need 2 million years to reach inside of the solar system [2]. The apparent brightness from the earth is regarded as a 11.4 class when this star reached its closest point to the sun [3]. It is thought that the event that a fixed star comes close to the solar system to distance equal to the ショルツ star 70,000 years ago is taking place at around one time of frequency for 9 million years [2].

Source

  1. ^ a b c d e f g "2MASS J07200325-0846499 - - Brown Dwarf Candidate". SIMBAD. February 21, 2015 reading.
  2. ^ a b c d e f g h i j k l m n o p q Mamajek, Eric E.; Barenfeld, Scott A.; Ivanov, Valentin D. (2015). "The Closest Known Flyby of a Star to the Solar System." The Astrophysical Journal 800 (1). arXiv: It is doi: 1502.04655 10.1088/2041-8205/800/1/L17. 
  3. ^ a b Mamajek, Eric. "FAQ". February 18, 2015 reading.
  4. ^ a b c d "Closest known flyby of star to our solar system: Dim star passed through Oort Cloud 70,000 years ago." ScienceDaily. (February 17, 2015). http://www.sciencedaily.com/releases/2015/02/150217114121.htm February 21, 2015 reading. 
  5. ^ ""The ショルツ star" which approached to great approach, オールト cloud 70,000 years ago". AstroArts (February 20, 2015). February 21, 2015 reading.
  6. ^ "THE ONE HUNDRED NEAREST STAR SYSTEMS." RECONS (Research Consortium On Nearby Stars). February 18, 2015 reading.

This article is taken from the Japanese Wikipedia ショルツ star

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